In Sections TheCircularFunctionsSineandCosine, TheOtherCircularFunctions and most recently TheInverseTrigonometricFunctions, we solved some basic equations involving the trigonometric functions. Below we summarize the techniques we’ve employed thus far. Note that we use the neutral letter ‘\(u\)’ as the argument of each circular function for generality.

Strategies for Solving Basic Equations Involving the Circular Functions
  • To solve \(\cos (u) = c\) or \(\sin (u) = c\) for \(-1 \leq c \leq 1\), first solve for \(u\) in the interval \([0,2\pi )\) and add integer multiples of the period \(2\pi \). If \(c < -1\) or of \(c > 1\), there are no real solutions.
  • To solve \(\sec (u) = c\) or \(\csc (u) = c\) for \(c \leq -1\) or \(c \geq 1\), convert to cosine or sine, respectively, and solve as above. If \(-1 < c < 1\), there are no real solutions.
  • To solve \(\tan (u) = c\) for any real number \(c\), first solve for \(u\) in the interval \(\left (-\frac {\pi }{2}, \frac {\pi }{2}\right )\) and add integer multiples of the period \(\pi \).
  • To solve \(\cot (u) = c\) for \(c \neq 0\), convert to tangent and solve as above. If \(c = 0\), the solution to \(\cot (u) = 0\) is \(u = \frac {\pi }{2} + \pi k\) for integers \(k\).

Using the above guidelines, we can comfortably solve \(\sin (x) = \frac {1}{2}\) and find the solution \(x = \frac {\pi }{6} + 2\pi k\) or \(x = \frac {5\pi }{6} + 2\pi k\) for integers \(k\). But how do we solve the related equation \(\sin (3x) = \frac {1}{2}\)?

Since this equation has the form \(\sin (u) = \frac {1}{2}\), we know the solutions take the form \(u= \frac {\pi }{6} + 2\pi k\) or \(u = \frac {5\pi }{6} + 2\pi k\) for integers \(k\). Since the argument of sine here is \(3x\), we have \(3x= \frac {\pi }{6} + 2\pi k\) or \(3x = \frac {5\pi }{6} + 2\pi k\).

To solve for \(x\), we divide both sides of these equations by \(3\), and obtain \(x = \frac {\pi }{18} + \frac {2\pi }{3} k\) or \(x = \frac {5\pi }{18} + \frac {2\pi }{3}k\) for integers \(k\). This is the technique employed in the example below.

If one looks closely at the equations and solutions in Example TrigEqnEx1, an interesting relationship evolves between the frequency of the circular function involved in the equation and how many solutions one can expect in the interval \([0, 2\pi )\). This relationship is explored in Exercise frequencynumberconnection.

Each of the problems in Example TrigEqnEx1 featured one circular function. If an equation involves two different circular functions or if the equation contains the same circular function but with different arguments, we will need to employ identities and Algebra to reduce the equation to the same form as those given on page 1. We demonstrate these techniques in the following example.

We repeat here the advice given when solving systems of nonlinear equations in section NonLinearEquations – when it comes to solving equations involving the circular functions, it helps to just try something.

Next, we focus on solving inequalities involving the circular functions. Since these functions are continuous on their domains, we may use the sign diagram technique we’ve used in the past to solve the inequalities.

Our next example puts solving equations and inequalities to good use – finding domains of functions.

In our next example, we solve equations and inequalities involving the inverse circular functions.

1 Harmonic Motion

One of the major applications of the circular functions (sinusoids in particular!) in Science and Engineering is the study of harmonic motion, We close this chapter with a brief foray into this topic since it pulls together many important concepts from both Chapters ?? and ??. The equations for harmonic motion can be used to describe a wide range of phenomena, from the motion of an object on a spring, to the response of an electronic circuit. In this subsection, we restrict our attention to modeling a simple spring system. Before we jump into the Mathematics, there are some Physics terms and concepts we need to discuss.

In Physics, ‘mass’ is defined as a measure of an object’s resistance to straight-line motion whereas ‘weight’ is the amount of force (pull) gravity exerts on an object. An object’s mass cannot change, while its weight could change. An object which weighs 6 pounds on the surface of the Earth would weigh 1 pound on the surface of the Moon, but its mass is the same in both places. In the English system of units, ‘pounds’ (lbs.) is a measure of force (weight), and the corresponding unit of mass is the ‘slug’. In the SI system, the unit of force is ‘Newtons’ (N) and the associated unit of mass is the ‘kilogram’ (kg).

We convert between mass and weight using the formula \(w = mg\). Here, \(w\) is the weight of the object, \(m\) is the mass and \(g\) is the acceleration due to gravity. In the English system, \(g = 32 \frac {\text {feet}}{\text {second}^2}\), and in the SI system, \(g = 9.8\frac {\text {meters}}{\text {second}^2}\). Hence, on Earth a mass of 1 slug weighs 32 lbs. and a mass of 1 kg weighs 9.8 N. Suppose we attach an object with mass \(m\) to a spring as depicted below.

The weight of the object will stretch the spring. The system is said to be in ‘equilibrium’ when the weight of the object is perfectly balanced with the restorative force of the spring. How far the spring stretches to reach equilibrium depends on the spring’s ‘spring constant’. Usually denoted by the letter \(k\), the spring constant relates the force \(F\) applied to the spring to the amount \(d\) the spring stretches in accordance with Hooke’s Law \(F = kd\).

If the object is released above or below the equilibrium position, or if the object is released with an upward or downward velocity, the object will bounce up and down on the end of the spring until some external force stops it. If we let \(x(t)\) denote the object’s displacement from the equilibrium position at time \(t\), then \(x(t) = 0\) means the object is at the equilibrium position, \(x(t) < 0\) means the object is above the equilibrium position, and \(x(t) > 0\) means the object is below the equilibrium position. The function \(x(t)\) is called the ‘equation of motion’ of the object.

If we ignore all other influences on the system except gravity and the spring force, then Physics tells us that gravity and the spring force will battle each other forever and the object will oscillate indefinitely. In this case, we describe the motion as ‘free’ (meaning there is no external force causing the motion) and ‘undamped’ (meaning we ignore friction caused by surrounding medium, which in our case is air).

The following theorem, which comes from Differential Equations, gives \(x(t)\) as a function of the mass \(m\) of the object, the spring constant \(k\), the initial displacement \(x_0\) of the object and initial velocity \(v_0\) of the object.

As with \(x(t)\), \(x_0 = 0\) means the object is released from the equilibrium position, \(x_0 < 0\) means the object is released above the equilibrium position and \(x_0>0\) means the object is released below the equilibrium position. As far as the initial velocity \(v_0\) is concerned, \(v_0 =0 \) means the object is released ‘from rest,’ \(v_0<0\) means the object is heading upwards and \(v_0>0\) means the object is heading downwards.

It is a great exercise in ‘dimensional analysis’ to verify that the formulas given in Theorem 1 work out so that \(\omega \) has units \(\frac {1}{s}\) and \(A\) has units ft. or m, depending on which system we choose.

Though beyond the scope of this course, it is possible to model the effects of friction and other external forces acting on the system.

While we may not have the Physics and Calculus background to derive equations of motion for these scenarios, we can certainly analyze them. We examine three cases in the following example.

Our last examples use the tools of this section along with those developed in Section ??.

We’ll continue our work with \(f(x) = 2 \sin (x) - \sin (2x)\) from Example 8 in Exercise ??.

We’ll revisit \(f(x) = x-2\cos (x)\) from Example 9 in Exercise ??. Speaking of Exercises …